Dynamical and static solutions to R=0 scalar-tensor theory

dc.contributor.authorAzreg-Ainou, Mustapha
dc.date.accessioned2021-04-28T06:30:57Z
dc.date.available2021-04-28T06:30:57Z
dc.date.issued2020
dc.description.abstractWe consider the most cosmologically interesting and relevant case of scalar-tensor theory (STT) and derive new normal and phantom, dynamical and static, solutions. We determine the Bianchi I Kasner exponents and show that the dynamical solutions are heteroclinic orbits connecting two singularities. Approaching the singularities, a purely transverse expansion (no radial expansion or collapse) may occur. Copyright (C) EPLA, 2020en_US
dc.identifier.issn0295-5075en_US
dc.identifier.issue6en_US
dc.identifier.scopus2-s2.0-85089853684en_US
dc.identifier.urihttp://hdl.handle.net/11727/5786
dc.identifier.volume130en_US
dc.identifier.wos000577009400002en_US
dc.language.isoengen_US
dc.relation.isversionof10.1209/0295-5075/130/60003en_US
dc.relation.journalEPLen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergien_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titleDynamical and static solutions to R=0 scalar-tensor theoryen_US
dc.typeArticleen_US

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